{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:2LBLPDKX2MZB2LNQKEXF267J4C","short_pith_number":"pith:2LBLPDKX","schema_version":"1.0","canonical_sha256":"d2c2b78d57d3321d2db0512e5d7be9e0a13ce0457a61d4f762142a47e43d58f4","source":{"kind":"arxiv","id":"1404.7014","version":1},"attestation_state":"computed","paper":{"title":"The PEP Survey: Infrared Properties of Radio-Selected AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"B. Magnelli, D. Lutz, D. Rosario, E. Le Floc'h, F. Pozzi, L. Riguccini, M. Magliocchetti, P. Santini, S. Berta","submitted_at":"2014-04-28T14:49:47Z","abstract_excerpt":"By exploiting the VLA-COSMOS and the Herschel-PEP surveys, we investigate the Far Infrared (FIR) properties of radio-selected AGN. To this purpose, from VLA-COSMOS we considered the 1537, F[1.4 GHz]>0.06 mJy sources with a reliable redshift estimate, and sub-divided them into star-forming galaxies and AGN solely on the basis of their radio luminosity. The AGN sample is complete with respect to radio selection at all z<~3.5. 832 radio sources have a counterpart in the PEP catalogue. 175 are AGN. Their redshift distribution closely resembles that of the total radio-selected AGN population, and e"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1404.7014","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-28T14:49:47Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"334ef8297a10c9ee99dbb87919f4b94f18e896fca7c5f787158867c73217fa69","abstract_canon_sha256":"45e87815a10a42de1af701e40d118639b6752a52d6ae2da9ea6fcfe0dabeb017"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:22.629105Z","signature_b64":"8MU33v/Zvd+VVgd6MFMxIZZVRYeRfUhCEKr/K8ANiIXDyu22N07YzginMHp+6WktYqPwKebVLzhVOCLeZoIXDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d2c2b78d57d3321d2db0512e5d7be9e0a13ce0457a61d4f762142a47e43d58f4","last_reissued_at":"2026-05-18T01:43:22.628556Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:22.628556Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The PEP Survey: Infrared Properties of Radio-Selected AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"B. Magnelli, D. Lutz, D. Rosario, E. Le Floc'h, F. Pozzi, L. Riguccini, M. Magliocchetti, P. Santini, S. Berta","submitted_at":"2014-04-28T14:49:47Z","abstract_excerpt":"By exploiting the VLA-COSMOS and the Herschel-PEP surveys, we investigate the Far Infrared (FIR) properties of radio-selected AGN. To this purpose, from VLA-COSMOS we considered the 1537, F[1.4 GHz]>0.06 mJy sources with a reliable redshift estimate, and sub-divided them into star-forming galaxies and AGN solely on the basis of their radio luminosity. The AGN sample is complete with respect to radio selection at all z<~3.5. 832 radio sources have a counterpart in the PEP catalogue. 175 are AGN. Their redshift distribution closely resembles that of the total radio-selected AGN population, and e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.7014","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1404.7014","created_at":"2026-05-18T01:43:22.628639+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.7014v1","created_at":"2026-05-18T01:43:22.628639+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.7014","created_at":"2026-05-18T01:43:22.628639+00:00"},{"alias_kind":"pith_short_12","alias_value":"2LBLPDKX2MZB","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_16","alias_value":"2LBLPDKX2MZB2LNQ","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_8","alias_value":"2LBLPDKX","created_at":"2026-05-18T12:28:11.866339+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C","json":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C.json","graph_json":"https://pith.science/api/pith-number/2LBLPDKX2MZB2LNQKEXF267J4C/graph.json","events_json":"https://pith.science/api/pith-number/2LBLPDKX2MZB2LNQKEXF267J4C/events.json","paper":"https://pith.science/paper/2LBLPDKX"},"agent_actions":{"view_html":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C","download_json":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C.json","view_paper":"https://pith.science/paper/2LBLPDKX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.7014&json=true","fetch_graph":"https://pith.science/api/pith-number/2LBLPDKX2MZB2LNQKEXF267J4C/graph.json","fetch_events":"https://pith.science/api/pith-number/2LBLPDKX2MZB2LNQKEXF267J4C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C/action/storage_attestation","attest_author":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C/action/author_attestation","sign_citation":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C/action/citation_signature","submit_replication":"https://pith.science/pith/2LBLPDKX2MZB2LNQKEXF267J4C/action/replication_record"}},"created_at":"2026-05-18T01:43:22.628639+00:00","updated_at":"2026-05-18T01:43:22.628639+00:00"}